These general trends have been also confirmed by following simulation campaigns [1]}, [2]}, [3]}.
In addition to consistent results on the relation between AGN feedback effects and the enrichment level at large distances from the center (i.e. beyond \(\sim 0.3\,R_{500}\) ), these recent simulations also finally reproduced the diversity of thermal and chemical properties found in the core (\(\lesssim 0.1\times R_{500}\) ) of observed systems [1]}, [5]}.
Some differences, e.g. on the metallicity profile normalization and thus on the global enrichment level, is nonetheless still present depending on the specific set of simulations analysed [6]}, and consequently on the set of stellar yields and supernova rates adopted.
In addition, the modelling of dust and metal spreading within cosmological simulations can further impact the details of the spatial distribution of metals that remain in the gaseous phase, for which further dedicated studies are needed.
